File:Constellations from Milky Way center.png
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| Description |
English: This image was created from the incredible free program Celestia; its images are available under the GPL. This is a view in the direction of Sol from the approximate center of the Milky Way. The sun's apparent magnitude is around 20 or so at this distance. Lavender lines connect the constellations. — Knowledge Seeker দ 08:24, 25 February 2006 (UTC) |
| Date | 25 February 2006 (original upload date) |
| Source | Transferred from en.wikipedia to Commons by IngerAlHaosului using CommonsHelper. |
| Author | The original uploader was Knowledge Seeker at English Wikipedia. |
| Permission (Reusing this file) |
GPL. |
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This work is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 2 of the License, or any later version. This work is distributed in the hope that it will be useful, but without any warranty; without even the implied warranty of merchantability or fitness for a particular purpose. See version 2 and version 3 of the GNU General Public License for more details. |
Original upload log edit
The original description page was here. All following user names refer to en.wikipedia.
- 2006-02-25 08:39 Knowledge Seeker 1920×1109× (360026 bytes) This image was created from the incredible free program Celestia; its images are available under the GPL. This is a view in the direction of Sol from the approximate center of the Milky Way. Earth. Lavender lines connect the constellations. — Knowledge
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 12:04, 15 January 2010 | | 1,920 × 1,109 (352 KB) | File Upload Bot (Magnus Manske) (talk | contribs) | {{BotMoveToCommons|en.wikipedia|year={{subst:CURRENTYEAR}}|month={{subst:CURRENTMONTHNAME}}|day={{subst:CURRENTDAY}}}} {{Information |Description={{en|This image was created from the incredible free program Celestia; its images are available under the GP |
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